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The chemical evolution of galaxies at high redshift

L. J. Smith·M. Pettini·D. L. King·R. W. Hunstead
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Abstract

Observations of absorption lines in the spectra of distant QSOs offer a new approach for tracking the evolution of normal galaxies from early epochs to the present day. The damped Ly alpha systems are particularly suitable for measuring the properties of what are likely to be the progenitors of present-day luminous galaxies. We have recently concluded a long-term survey of 30 damped absorbers (including eight from the literature) aimed at measuring the metallicity and dust content of the universe from redshift z = 3.39 to 0.69. The major conclusions are that the epoch of chemical enrichment in galaxies may have begun at z = 2.5-3--corresponding to a look-back time of 14 Gyr--and that at z = 2 the typical metallicity was 1/15 of solar. There is clear evidence for the presence of interstellar dust at z = 2, although several high-redshift galaxies, particularly the most metal-poor, appear to be essentially dust-free. We discuss the nature of the damped Ly alpha galaxies in the light of these and other new results.

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L. J. Smith, M. Pettini, D. L. King, R. W. Hunstead. 1996-01-26. The chemical evolution of galaxies at high redshift. https://arxiv.org/abs/astro-ph/9601153

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